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Nuclear Incompressibility
The isoscalar incompressibility of infinite nuclear matter is defined by
the well-known formula [1]
|
(29) |
where is the saturation density of nuclear matter. Of
course,
cannot be directly measured; however, by using
Eq. (29) it can be calculated from theoretical equation of
state or it can be indirectly estimated from measurements
of monopole excitations of finite nuclei.
The incompressibility of finite nucleus, , is defined by its scaling-model
relation [28] to
the centroid of the giant monopole resonance (GMR),
, as
|
(30) |
where
is the average square radius of the nucleus.
Eq. (30) is derived under the assumption that most of the monopole
strength is concentrated within one dominant peak, see Ref. [1].
The centroid of the GMR can be extracted from its strength function as
the ratio of the first and zero moments, that is,
|
(31) |
There exist several alternative ways to extract
through
different moments of the strength function, such as
or
. However, they are more sensitive
to details of the strength function and thus less appropriate
for studies of the incompressibility.
In analogy to the Weizsäcker formula for the nuclear masses,
one can introduce [1] a similar relation for nuclear incompressibilities,
Similarly as in the liquid-drop model, we refer to , , ,
, and as the volume, surface, symmetry, surface-symmetry,
and Coulomb incompressibility parameters, respectively. By adjusting
these parameters to the incompressibilities , calculated in finite nuclei
from Eqs. (30) and (31),
we can obtain an estimate of the infinite-matter incompressibility as
.
Next: Results
Up: Giant Monopole Resonances and
Previous: Separable Pairing Interaction
Jacek Dobaczewski
2012-02-28